EPJ Web Conf.
Volume 197, 2019Atmospheric Monitoring for High Energy Astroparticle Detectors (AtmoHEAD) 2018
|Number of page(s)||4|
|Section||Analysis Techniques and Instruments|
|Published online||15 January 2019|
Atmospheric Monitoring at a Cosmic Ray Observatory - a long-lasting endeavour
Karlsruhe Institute of Technology (KIT), Institute for Nuclear Physics,
2 Observatorio Pierre Auger, Av. San Martin Norte 304, 5613 Malargüe, Argentina
Published online: 15 January 2019
The Pierre Auger Observatory for detecting ultrahigh energy cosmic rays has been founded in 1999. After a main planning and construction phase of about five years, the regular data taking started in 2004, but it took another four years until the full surface detector array was deployed. In parallel to the main detectors of the Observatory, a comprehensive set of instruments for monitoring the atmospheric conditions above the array was developed and installed as varying atmospheric conditions influence the development and detection of extensive air showers. The multitude of atmospheric monitoring installations at the Pierre Auger Observatory will be presented as well as the challenges and efforts to run such instruments for several decades.
© The Authors, published by EDP Sciences, 2019
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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